A dataset provided by the European Space Agency

Name: In-orbit measurement of the XMM telescope vignetting function
Published: 2000-03-09T00:00:00Z

Proposal ID	009501
Title	In-orbit measurement of the XMM telescope vignetting function
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095010901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095011101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095011301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095011401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095011501
DOI	https://doi.org/10.5270/esa-376kiza
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	CAL- Observations of the compact cluster of galaxies A496 at different off-axisangles will provide changes in count rates for different energy bands. Thesewill be used to derive the vignetting function of the XMM telescopes indifferent energy bands.
Publications	XMM-Newton observations of the cluster of galaxies Abell 496. Measurements of the elemental abundances in the intracluster medium \|Tamura T. Bleeker J. A. M. et al. \| A&A \| 379-107 \| 2001 \| 2001A&A...379..107T \| http://ui.adsabs.harvard.edu/#abs/2001A&A...379..107T Cold fronts in galaxy clusters \|Ghizzardi S. Rossetti M. \| A&A \| 516-32 \| 2010 \| 2010A&A...516A..32G \| http://ui.adsabs.harvard.edu/#abs/2010A&A...516A..32G The cool-core bias in X-ray galaxy cluster samples. I. Method and application to HIFLUGCS \|Eckert D. Molendi S. \| A&A \| 526-79 \| 2011 \| 2011A&A...526A..79E \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A..79E Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F X-Ray Morphological Analysis of the Planck ESZ Clusters \|Lovisari Lorenzo Forman William R. et al. \| ApJ \| 846-51 \| 2017 \| 2017ApJ...846...51L \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...846...51L Charge exchange in galaxy clusters \|Gu Liyi Mao Junjie et al. \| A&A \| 611-26 \| 2018 \| 2018A&A...611A..26G \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..26G X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton \|Lovisari Lorenzo Schellenberger Gerrit et al. \| ApJ \| 892-102 \| 2020 \| 2020ApJ...892..102L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...892..102L Comparing different mass estimators for a large subsample of the Planck-ESZ clusters \|Lovisari L. Ettori S. et al. \| A&A \| 644-78 \| 2020 \| 2020A&A...644A..78L \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A..78L The thermalization of massive galaxy clusters \|Sereno Mauro Lovisari Lorenzo et al. \| MNRAS \| 507-5214 \| 2021 \| 2021MNRAS.507.5214S \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.5214S Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters \|Wicker R. Douspis M. et al. \| A&A \| 674-48 \| 2023 \| 2023A&A...674A..48W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A..48W From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2000-03-13T10:00:29Z/2000-03-15T01:31:26Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2000-03-09T00:00:00Z
Last Update	2025-01-27
Keywords	"energy bands", "count rates", "axis angles", "vignetting function", "orbit measurement", "xmm telescopes", "compact cluster", "galaxy a496", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2000, 'In-orbit measurement of the XMM telescope vignetting function', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-376kiza